Download OCR G485 Definitions

OCR G485 Definitions
Module 1 - Electric and Magnetic Fields
Coulomb’s Law - The force between two electric charges is proportional to the product of
the charges and inversely proportional to the square of the distance between them.
Electric Field Strength - Force per unit positive charge
Magnetic Flux Density - A measure of the strength of a magnetic field, defined by:
where B = magnetic flux density (T), I = current in the wire (A), l = length of the
wire (m), F = the force experienced (N) and θ = the angle between the wire and the field.
Tesla - The unit of magnetic flux density, when a wire of length 1m carrying a current of 1A
perpendicular to the field experiences a force of 1N.
Magnetic Flux - The product of magnetic flux density, B and the projection of area, A onto a
surface at right angles to the flux. Unit = Weber
Weber - One Weber is the unit of magnetic flux when a magnetic field of magnetic flux
density 1 Tesla, passes at right angles through an area of 1m2.
Magnetic Flux Linkage - the product of the magnetic flux and the number of turns on the
coil. Unit = Weber turns.
Faradays Law of E.M. Induction - The magnitude of the induced e.m.f. is equal to the rate at
which magnetic flux is cut.
For a coil this becomes: The induced e.m.f. is equal to the rate of change of flux linkage.
Lenz’s Law - The direction of the induced e.m.f. is such that it opposes the change causing it.
Module 2 - Capacitance
Capacitance - Charge stored per unit potential difference.
Farad - One Coulomb per volt.
Time Constant - The time taken for the voltage or charge to drop to 37% of its original
value.
Module 3 - Nuclear Physics
Proton Number, Z - The number of protons in a nucleus.
Nucleon Number, A - The number of nucleons in any nucleus.
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Isotopes - Two nuclides (a nucleus with a distinct number of protons and neutrons) with the
same number of protons but different numbers of neutrons.
Fundamental Particles - Particles which cannot be broken down into smaller components.
Activity - The number of radioactive decays per unit time. Unit = Becquerels.
N.B. 1 Bq = 1s-1 (I decay per second.)
Decay Constant, λ - The fraction of atoms decaying in unit time.
Half-life - The average time taken for the activity of a radioactive source to decrease to one
half of its original value. OR The time taken for the number of radioactive nuclei to
decrease by ½.
Binding Energy - The work done against the electrostatic force in assembling a nucleus from
its individual protons and neutrons.
Module 4 - Medical Imaging
Intensity (of a beam of X-Rays) - Power per unit Cross-Sectional Area.
Module 5 - Modelling the Universe
Astronomical Unit (AU) - the average distance from the centre of the Earth to the centre of
the Sun. 1 AU = 1.496 x 1011 m
Parsec (PC) - The distance when a baseline of length 1 AU when the angle is one second of
an arc (that angle is 1/3600 of a degree.) 1 Pc = 3.086 x 1016 m
Light-Year (ly) - The distance light travels through a vacuum in a year. 1 ly = 9.461 x 1015 m
Olber’s Paradox - If the universe was infinite, there would be stars in every direction; so it
wouldn’t be dark at night.
Conclusions:
•
•
•
either the universe is not infinite
or the stars are not uniformly distributed
or the universe is not static
(or two or all of these might be true.)
Hubble’s Law - The speed of recession of a galaxy is directly proportional to its distance
from Earth.
Conclusions: The universe is expanding - everything is moving away from everything else,
not just moving away from Earth.
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Cosmological Principle - On a large scale, the universe is homogenous (of uniform density) and
isotropic (the same in all directions.) Providing a large enough volume is considered.
Critical Density - The average density of the universe, above which the universe will collapse (closed
universe) and below which the universe will expand forever (open universe.)
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